M. E. Jarvis
Max Planck Society
10 Papers
13 Citations
M. E. Jarvis is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Quasar. The author has an hindex of 4, co-authored 10 publications. Previous affiliations of M. E. Jarvis include Ludwig Maximilian University of Munich & European Southern Observatory.
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Papers
Extreme ionised outflows are more common when the radio emission is compact in AGN host galaxies
TL;DR: In this paper, radio observations for a subset of targets in this luminosity range reveal that radio jets and lobes are prevalent, and suggest that compact jets might be responsible for the stronger outflows in the wider sample.
Outflows in the radio-intermediate quasar III Zw 2: a polarization study with the EVLA and uGMRT
S. Silpa,Preeti Kharb,Christopher Harrison,Luis C. Ho,M. E. Jarvis,M. E. Jarvis,M. E. Jarvis,C. H. Ishwara-Chandra,Biny Sebastian +8 more
TL;DR: In this paper, a radio-intermediate quasar, III Zw 2, was studied at a redshift of 0.0893 with the upgraded Giant Metrewave Radio Telescope (uGMRT) at 685 MHz and the Karl Jansky Very Large Array (VLA) at 5 and 34 GHz.
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Extreme ionised outflows are more common when the radio emission is compact in AGN host galaxies
TL;DR: In this article, the authors show that radio jets and lobes are prevalent for the highest radio luminosity bin of log[L(1.4GHz)/(W/Hz)]=23.5-24.5 where the AGN dominated the radio emission; specifically, >1000 km/s components are almost four times more likely when the radio emissions are compact in this subsample.
The radio structure of the narrow-line Seyfert 1 Mrk 783 with VLBA and e-MERLIN
Enrico Congiu,Enrico Congiu,Preeti Kharb,Andrea Tarchi,Marco Berton,Marco Berton,Alessandro Caccianiga,Sina Chen,L. Crepaldi,F. Di Mille,Emilia Järvelä,M. E. Jarvis,M. E. Jarvis,M. E. Jarvis,G. La Mura,A. Vietri +15 more
TL;DR: In this article, radio and optical observations of the narrow-line Seyfert 1 galaxy Mrk 783 were performed with the e-MERLIN interferometer to confirm the presence of diffuse emission previously observed.
Establishing the impact of powerful AGN on their host galaxies
TL;DR: In this paper, the role of active galactic nuclei (AGN) during the formation of galaxies remains one of the greatest challenges of galaxy formation theory and the physical drivers of ionised outflows and observational signatures of the impact by jets/outflows on star formation and molecular gas content in AGN host galaxies are investigated.
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